The Frequency Drift and Time Splitting of Decameter Solar Radio Bursts
Ch. V. Sastry
Abstract
Ch. V. Sastry
Abstract
The frequency drift and time splitting of solar radio bursts are observed \nwith a multi-channel radiometer and a polarimeter at frequencies around 25 \nMHz. It is found that a majority of noise storm bursts have drift rates \nbetween + 1.0 and -1.0 MHz/sec. Two types of unusual bursts with frequency \ndrift are described. The two components of a double burst are found to be \npolarized to the same degree and in the same sense.
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The frequency drift and time splitting of solar radio bursts are observed \nwith a multi-channel radiometer and a polarimeter at frequencies around 25 \nMHz. It is found that a majority of noise storm bursts have drift rates \nbetween + 1.0 and -1.0 MHz/sec. Two types of unusual bursts with frequency \ndrift are described. The two components of a double burst are found to be \npolarized to the same degree and in the same sense.
Key concepts: Solar radio, Physics, Astrophysics, Astronomy, Solar physics, Solar flare